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Het OWA, het open archief van het Waterbouwkundig Laboratorium heeft tot doel alle vrij toegankelijke onderzoeksresultaten van dit instituut in digitale vorm aan te bieden. Op die manier wil het de zichtbaarheid, verspreiding en gebruik van deze onderzoeksresultaten, alsook de wetenschappelijke communicatie maximaal bevorderen.
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Mercury's crustal thickness correlates with lateral variations in mantle melt production
Beuthe, M.; Charlier, B.; Namur, O.; Rivoldini, A.; Van Hoolst, T. (2020). Mercury's crustal thickness correlates with lateral variations in mantle melt production. Geophys. Res. Lett. 47(9): e2020GL087261. https://hdl.handle.net/10.1029/2020GL087261
In: Geophysical Research Letters. American Geophysical Union: Washington. ISSN 0094-8276; e-ISSN 1944-8007, meer
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| Author keywords |
Mercury; crust thickness; volcanism; mantle melting |
| Abstract |
Over the first billion years of Mercury's history, mantle melting and surface volcanism produced a secondary magmatic crust varying spatially in composition and mineralogy. By combining geochemical mapping from MESSENGER with laboratory experiments on partial melting, we translate the surface mineralogy into lateral variations of surface density and calculate the degree of mantle melting required to produce surface rocks. If lateral density variations extend through the whole crust, the local crustal thickness correlates well with the degree of mantle melting. Low-degree mantle melting produced a thin crust below the northern volcanic plains (19±3 km), whereas high-degree melting produced the thickest crust in the ancient high-Mg region (50±12 km), refuting the hypothesis of an impact origin for that region. The thickness-melting correlation has also been observed for the oceanic crust on Earth and might be a common feature of secondary crust formation on terrestrial planets. |
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